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Period Changes of Ten Eclipsing Variable Stars

Published online by Cambridge University Press:  25 April 2016

Kyu-Dong Oh*
Affiliation:
Department of Earth Sciences, Chonnam National University, Kwangju, Korea

Abstract

We examine the period variations of ten eclipsing binary stars and from the combined result, attempt to construct a physical explanation for their behaviour.

Type
Galactic and Stellar
Copyright
Copyright © Astronomical Society of Australia 1991

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References

Alduseva, V. Ya., 1986, Pis’ma Astron. Zh., 12, 212.Google Scholar
Bames, R., 1974, Publ. Astron. Soc. Pac., 86, 195.Google Scholar
Biermann, P. and Hall, D. S., 1973, Astron. Astrophys., 27, 249.Google Scholar
Hall, D. S. and Neff, S. G., 1979, Acta. Astron., 29, 641.Google Scholar
Prikhod’ko, A. E., 1961, A. ZA., 38, 937.Google Scholar
Strupat, W., 1987, Astron. Astrophys., 185, 150.Google Scholar
Taranova, O. G., 1987, Pis’ma Astron. Zh., 13, 502.Google Scholar
Wood, F.B., 1950, Astrophys. J., 112, 196.CrossRefGoogle Scholar